Download Neutrino Oscillations and Their Origin: Proceedings of the by Y. Suzuki, Y. Fukuda, T. Takeuchi, T. Mori, T. Yoshida PDF

By Y. Suzuki, Y. Fukuda, T. Takeuchi, T. Mori, T. Yoshida

This paintings covers themes akin to the newest sun neutrino leads to super-kamiokande, susceptible present in deuterium, proton decay within the semi-simple unification version, and 4 puzzles of neutrino blending.

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18. 19. 20. 21. 22. 23. 24. 25. 26. 27. G. Adelberger et al, Rev. Mod. Phys. 70, 1265 (1998). R. Ahmad, et al, Phys. Rev. Lett. 87, 071301 (2001). M. Altmann, et al, Phys. Lett. B 490, 16 (2000). N. H. Pinsonneault, Rev. Mod. Phys. 67, 781 (1995). N. H. Pinsonneault, and S. Basu, ApJ 555, 990 (2001). S. Basu, MNRAS 289, 719 (1998). S. M. Antia, MNRAS 287, 189 (1997). T. Cleveland et al, ApJ 496, 505 (1998). R. Elliott, A&A 334, 703 (1998). Y. Fukuda et al, Phys. Rev. Lett. 86, 5651 (2001). N. Gavrin, Nuclear.

The SNO Collaboration, Phys. Lett. B 194, 321 (1987), and references therein. 2. Q. , Phys. Rev. Lett. 87, 071301 (2001). 3. N. Tatara, Y. Kohyama and K. Kubodera, Phys. Rev. C 42, 1694 (1990); S. Ying, W. C. Haxton and E. M. Henley, Phys. Rev. C 45, 1982 (1992); for a review, see K. Kubodera and S. Nozawa, Int. J. Mod. Phys. E 3, 101 (1994). 29 4. S. Nakamura, T. Sato, V. Gudkov and K. Kubodera, Phys. Rev. C 63, 034617 (2001). 5. For a review, see U. van Kolck, Prog. Part. Nucl. R. Beane et al, in "At the Frontiers of Particle Physics - Handbook of QCD", ed.

Acknowledgments This analysis relies crucially on Super-Kamiokande data. The author acknowledges the extensive help and cooperation of the Super-Kamiokande collaboration as well as the Kamioka Mining and Smelting Company. S. S. National Science Foundation. Appendix: Fitting Method To estimate and limit oscillation parameters, a \2 describing the shape of the SK zenith spectrum is extended to take into account the measured neutrino interaction rates by various experiments. " (due to hep neutrinos) in energy bin i and zenith-angle bin z are calculated.

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